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Table 4

NGC 104: ephemerides and main characteristics of the variable stars in the field of this globular cluster.

Var id RA Dec Epoch P I median A i′ + z N Type
J2000 J2000 HJD d mag mag

PC1-V12 00:24:05.921 72:04:45.20 15.62 1.10 149 NC
WF2-V34 00:24:08.406 72:04:35.91 10.98 0.03 139 L
LW10 00:24:02.490 72:05:07.45 9.60 0.24 108 L
LW11 00:24:03.145 72:04:50.60 2 456 920.7253 19.37(8) 10.18 0.08 141 SR
LW12 00:24:03.982 72:05:10.06 9.57 0.09 41 L

EM1 00:24:03.065 72:04:55.02 2 456 491.9380 20.28(9) 10.26 0.05 145 SR
EM2 00:24:06.269 72:04:45.36 2 456 530.7986 31.50(22) 9.98 0.08 140 SR
EM3 00:24:08.310 72:04:50.69 2 456 847.9667 33.41(24) 10.07 0.05 134 SR
EM4 00:24:07.203 72:04:46.45 2 456 498.9086 68.07(102) 13.89 0.14 149 SR
EM5 00:24:05.087 72:04:54.38 10.34 0.06 145 L
EM6 00:24:02.733 72:05:02.80 10.60 0.07 147 L
EM7 00:24:07.885 72:05:02.00 146 NC

Notes. Column 1 contains the id assigned to the variable star, Cols. 2 and 3 correspond to the right ascension and declination (J2000), Col. 4 shows the epoch used, Col. 5 shows the period, Col. 6 contains median of the data, Col. 7 shows the peak-to-peak amplitude in the light curve, Col. 8 contains the number of epochs and Col. 9 shows the classification of the variable. The numbers in parentheses indicate the uncertainty on the last decimal place of the period.

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